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A revised algorithm for calculating TiO2 from Clementine UWIS data: A synthesis of rock, soil, and remotely sensed TiO2 concentrations

Author
GILLIS, Jeffrey J1 ; JOLLIFF, Bradley L1 ; ELPHIC, Rick C2
[1] Department of Earth and Planetary Sciences, Washington University, St. Louis, Missouri, United States
[2] Space and Atmospheric Sciences, Los Alamos National Laboratory, Los Alamos, New Mexico, United States
Source

Journal of geophysical research. 2003, Vol 108, Num E2, pp 3.1-3.18 ; Analysis , Illustration , Table ; ref : 1 p.1/4

ISSN
0148-0227
Scientific domain
Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
Publisher
American Geophysical Union, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Albedo Algorithme Apollo 11 Basalte lunaire Composition Concentration Etalonnage Luna 16 Luna 24 Lune Mer lunaire Pouvoir réflecteur Regolithe Révision Site atterrissage Spectrométrie UV Titane Traitement donnée Distribution bimodale Programme Clementine Spectrométrie visible
Keyword (en)
albedo algorithms Apollo 11 lunar basalts composition concentration calibration Luna 16 Luna 24 Moon maria reflectance regolith revision landing sites ultraviolet spectroscopy titanium data processing
Keyword (es)
Albedo Algoritmo Apolo 11 Concentración Contraste Luna 16 Luna Mar lunar Poder reflector Regolito Revisión Lugar aterrizaje Espectrometría UV Titanio Tratamiento datos
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences / 001E01D Cosmochemistry. Extraterrestrial geology / 001E01D01 Extraterrestrial geology

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
14756713

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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